no code implementations • 5 Nov 2020 • R. D. Baldi, D. R. A. Williams, I. M. McHardy, R. J. Beswick, E. Brinks, B. T. Dullo, J. H. Knapen, M. K. Argo, S. Aalto, A. Alberdi, W. A. Baan, G. J. Bendo, S. Corbel, D. M. Fenech, J. S. Gallagher, D. A. Green, R. C. Kennicutt, H. -R. Klöckner, E. Körding, T. J. Maccarone, T. W. B. Muxlow, C. G. Mundell, F. Panessa, A. B. Peck, M. A. Pérez-Torres, C. Romero-Cañizales, P. Saikia, F. Shankar, R. E. Spencer, I. R. Stevens, E. Varenius, M. J. Ward, J. Yates
Together with the 103 targets of the first LeMMINGs data release, this represents a complete sample of 280 local active (LINER and Seyfert) and inactive galaxies HII galaxies and Absorption Line Galaxies, ALG).
Astrophysics of Galaxies High Energy Astrophysical Phenomena
1 code implementation • 5 Dec 2016 • G. Calderone, L. Nicastro, G. Ghisellini, M. Dotti, T. Sbarrato, F. Shankar, M. Colpi
Improving on a number of previous studies on AGN spectral analysis, QSFit fits all the components simultaneously, using an AGN continuum model which extends over the entire available spectrum, and is thus a probe of the actual AGN continuum whose estimates are scarcely influenced by localized features (e. g. emission lines) in the spectrum.
High Energy Astrophysical Phenomena
